Results 21 to 30 of about 84,846 (229)

Tähistaeval põhinevatest uskumustest III Vana-Hiina [PDF]

open access: yesMäetagused, 2002
The article concerns Chinese astral myths, calendar and astrology. Chinese creation myths concern also the creation of the Sun, Moon and stars. The heavenly bodies are constantly endangered by the sky dragon that now and then catches them, probably a ...
Enn Kasak
doaj  

Shocklets in the Comet Halley Plasma [PDF]

open access: yes, 2020
Dust acoustic (DA) waves evolving into shocklets are investigated in the Comet Halley plasma system relaxing to Maxwellian, Kappa and Cairns distributions. Here dynamics of dust is described by the fully nonlinear continuity and momentum equations. A set of two characteristic wave nonlinear equations is obtained and numerically solved to examine the DA
arxiv   +1 more source

A model for the common origin of Jupiter family and Halley type comets [PDF]

open access: yesEarth, Moon, and Planets, 2013, Volume 110, Issue 1-2, pp. 105-130, 2014
A numerical simulation of the Oort cloud is used to explain the observed orbital distributions and numbers of Jupiter-family and Halley-type short-period comets. Comets are given initial orbits with perihelion distances between 5 and 36 AU, and evolve under planetary, stellar and Galactic perturbations for 4.5 Gyr.
arxiv   +1 more source

THE EFFECT OF A TRANS-PLUTONIAN PLANET ON HALLEY'S COMET

open access: yes, 1972
An orbit and mass for a hypothetical trans-Plutonian planet is determined which reduces the residuals in the time of perihelion passage of Halley's comet at the seven apparitions from 1910 to 1456 by 93%.
J. L. Brady
semanticscholar   +1 more source

Collision probabilities of migrating small bodies and dust particles with planets [PDF]

open access: yesIAU Symp.263:41-44,2010, 2009
Probabilities of collisions of migrating small bodies and dust particles produced by these bodies with planets were studied. Various Jupiter-family comets, Halley-type comets, long-period comets, trans-Neptunian objects, and asteroids were considered. The total probability of collisions of any considered body or particle with all planets did not exceed
arxiv   +1 more source

The end states of long-period comets and the origin of Halley-type comets [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2016, 2016
We analyze a sample of 73 old long-period comets (LPCs) (orbital periods $200 < P < 1000$ yr) with perihelion distances $q < 2.5$ au, discovered in the period 1850-2014. We cloned the observed comets and also added fictitious LPCs with perihelia in the Jupiter's zone.
arxiv   +1 more source

Ion‐Scale Characteristics of the Martian Magnetic Pile‐Up Boundary Layer

open access: yesGeophysical Research Letters, Volume 52, Issue 3, 16 February 2025.
Abstract The Martian magnetic pile‐up boundary (MPB) delineates the interface between the magnetosheath and the induced magnetosphere, but its global ion‐scale characteristics remaining unclear. Utilizing a three‐dimensional Hall magnetohydrodynamic (MHD) model, this study aims to reveal the features of the MPB layer, including magnetic field, current ...
Shibang Li   +12 more
wiley   +1 more source

Chaotic Dynamics of Comet 1P/Halley; Lyapunov Exponent and Survival Time Expectancy [PDF]

open access: yes, 2014
The orbital elements of comet Halley are known to a very high precision, suggesting that the calculation of its future dynamical evolution is straightforward. In this paper we seek to characterize the chaotic nature of the present day orbit of comet Halley and to quantify the timescale over which its motion can be predicted confidently. In addition, we
arxiv   +1 more source

Seasonal and Local Time Variation in the Observed Peak of the Meteor Altitude Distributions by Meteor Radars

open access: yesJournal of Geophysical Research: Atmospheres, Volume 129, Issue 21, 16 November 2024.
Abstract Meteoroids of sub‐milligram sizes burn up high in the Earth's atmosphere and cause streaks of plasma trails detectable by meteor radars. The altitude at which these trails, or meteors, form depends on a number of factors including atmospheric density and the astronomical source populations from which these meteoroids originate.
E. C. M. Dawkins   +26 more
wiley   +1 more source

Waves and Instabilities in Saturn's Magnetosheath: 2. Dispersion Relation Analysis

open access: yesJournal of Geophysical Research: Space Physics, Volume 129, Issue 10, October 2024.
Abstract The WHAMP (Rönnmark, 1982, https://inis.iaea.org/search/search.aspx?orig_q=RN:14744092) and LEOPARD (Astfalk & Jenko, 2017, https://doi.org/10.1002/2016ja023522) dispersion relation solvers were used to evaluate the growth rate and scale size for mirror mode (MM) and ion cyclotron (IC) instabilities under plasma conditions resembling Saturn's ...
I. Cheng   +4 more
wiley   +1 more source

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